Towards understanding astrophysical effects of nuclear symmetry energy
Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared
goal of both nuclear physics and astrophysics. Except possible phase transitions, the density …
goal of both nuclear physics and astrophysics. Except possible phase transitions, the density …
Nucleon effective masses in neutron-rich matter
Various kinds of isovector nucleon effective masses are used in the literature to characterize
the momentum/energy dependence of the nucleon symmetry potential or self-energy due to …
the momentum/energy dependence of the nucleon symmetry potential or self-energy due to …
Skyrme interaction and nuclear matter constraints
This paper presents a detailed assessment of the ability of the 240 Skyrme interaction
parameter sets in the literature to satisfy a series of criteria derived from macroscopic …
parameter sets in the literature to satisfy a series of criteria derived from macroscopic …
Nuclear energy density optimization
We carry out state-of-the-art optimization of a nuclear energy density of Skyrme type in the
framework of the Hartree-Fock-Bogoliubov theory. The particle-hole and particle-particle …
framework of the Hartree-Fock-Bogoliubov theory. The particle-hole and particle-particle …
Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XII. Stiffness and stability of neutron-star matter
We construct three new Hartree-Fock-Bogoliubov (HFB) mass models, labeled HFB-19, HFB-
20, and HFB-21, with unconventional Skyrme forces containing t 4 and t 5 terms, ie, density …
20, and HFB-21, with unconventional Skyrme forces containing t 4 and t 5 terms, ie, density …
Density slope of the nuclear symmetry energy from the neutron skin thickness of heavy nuclei
Expressing explicitly the parameters of the standard Skyrme interaction in terms of the
macroscopic properties of asymmetric nuclear matter, we show in the Skyrme-Hartree-Fock …
macroscopic properties of asymmetric nuclear matter, we show in the Skyrme-Hartree-Fock …
Incompressibility in finite nuclei and nuclear matter
JR Stone, NJ Stone, SA Moszkowski - Physical Review C, 2014 - APS
The incompressibility (compression modulus) K 0 of infinite symmetric nuclear matter at
saturation density has become one of the major constraints on mean-field models of nuclear …
saturation density has become one of the major constraints on mean-field models of nuclear …
Combined constraints on the equation of state of dense neutron-rich matter from terrestrial nuclear experiments and observations of neutron stars
Within the parameter space of the equation of state (EOS) of dense neutron-rich matter
limited by existing constraints mainly from terrestrial nuclear experiments, we investigate …
limited by existing constraints mainly from terrestrial nuclear experiments, we investigate …
Analytical representations of unified equations of state for neutron-star matter
Context. An equation of state (EoS) of dense nuclear matter is a prerequisite for studies of
the structure and evolution of compact stars. A unified EoS should describe the crust and the …
the structure and evolution of compact stars. A unified EoS should describe the crust and the …
New relativistic effective interaction for finite nuclei, infinite nuclear matter, and neutron stars
We carry out the study of finite nuclei, infinite nuclear matter, and neutron star properties with
the newly developed relativistic force, the Institute of Physics Bhubaneswar-I (IOPB-I). Using …
the newly developed relativistic force, the Institute of Physics Bhubaneswar-I (IOPB-I). Using …